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  • 1
    Electronic Resource
    Electronic Resource
    Supernova Remnants (1972)
    Palo Alto, Calif. : Annual Reviews
    Annual Review of Astronomy and Astrophysics 10 (1972), S. 129-158 
    Details
    ISSN: 0066-4146
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
    Topics: Physics
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1146/annurev.aa.10.090172.001021
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  • 2
    Electronic Resource
    Electronic Resource
    QUASARS (1973)
    Oxford, UK : Blackwell Publishing Ltd
    Annals of the New York Academy of Sciences 224 (1973), S. 0 
    Details
    ISSN: 1749-6632
    Source: Blackwell Publishing Journal Backfiles 1879-2005
    Topics: Natural Sciences in General
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1111/j.1749-6632.1973.tb41435.x
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  • 3
    Electronic Resource
    Electronic Resource
    ASTROPHYSICAL EVIDENCE FOR STRONG MAGNETIC FIELDS (1975)
    Oxford, UK : Blackwell Publishing Ltd
    Annals of the New York Academy of Sciences 257 (1975), S. 0 
    Details
    ISSN: 1749-6632
    Source: Blackwell Publishing Journal Backfiles 1879-2005
    Topics: Natural Sciences in General
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1111/j.1749-6632.1975.tb36078.x
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  • 4
    Electronic Resource
    Electronic Resource
    Limit on the frequency of intergalactic supernovae (1977)
    [s.l.] : Nature Publishing Group
    Nature 265 (1977), S. 124-126 
    Details
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] Relevant data on the supernovae within 3? of the Coma cluster centre are collected in Table 1. Most of the data came from the list of Sargent et al4, except the data on SN 1976 (IA U Circular no. 2921, 1976; the radial velocity from ref. 5), and the type of the parent galaxy of SN 1962i (ref. 6). ...
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1038/265124a0
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  • 5
    Electronic Resource
    Electronic Resource
    Concluding Remarks (1999)
    Springer
    Astrophysics and space science 265 (1999), S. 569-572 
    Details
    ISSN: 1572-946X
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1023/A:1002172430009
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  • 6
    Electronic Resource
    Electronic Resource
    X-ray sources and the diffuse background (1970)
    Springer
    Astrophysics and space science 9 (1970), S. 185-192 
    Details
    ISSN: 1572-946X
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract Possible numbers of X-ray sources at various flux levels are considered and their contribution to the background evaluated. Our conclusions are: The mean spectrum of Quasi-Stellar Objects and the nuclei of Seyfert galaxies between optical and X-ray wavelengths is characterized by a spectral index well in excess of 1.0. These objects may make an important contribution to the soft X-ray background. Observations of Q.S.O. may allow a decisive test for the cosmological interpretation of the redshifts of the Q.S.O. With regard to galactic sources we find that few undetected sources of the Sgr-Sco type exist, that these sources are located in the immediate neighborhood of the galactic center and that they account for at least 80% of the total galactic source luminosity. However, many intrinsically much fainter galactic sources may exist.
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1007/BF00649964
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  • 7
    Electronic Resource
    Electronic Resource
    Close Pairs of QSOs (1974)
    [s.l.] : Nature Publishing Group
    Nature 247 (1974), S. 22-23 
    Details
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] The expected number of close pairs of QSOs is given by (nR2) p(〈m) (1) where NQ is the total number of QSOs whose redshifts have been determined, R (in arc s) is the 'region of interest' around any given QSO (or the maximum allowable separation for 'close' pairs), and p(〈w) is the total ...
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1038/247022a0
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  • 8
    Electronic Resource
    Electronic Resource
    Infrared Background from Seyfert Galaxies (1970)
    [s.l.] : Nature Publishing Group
    Nature 227 (1970), S. 586-587 
    Details
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] A class of objects with a present (2 = 0) space density po and luminosity L0 in relativistic models with zero pressure and zero cosmological constant fills the universe with radiation with an energy density given by6 Here q0 is the deceleration parameter and z is the maximum redshift after which ...
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1038/227586a0
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  • 9
    Electronic Resource
    Electronic Resource
    A Source of Energy for Radio Galaxies (1964)
    [s.l.] : Nature Publishing Group
    Nature 201 (1964), S. 803-804 
    Details
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] It would appear that in many sources the production of particles should continue for an appreciable time. In Cent. A and Vir. A, for example, the existence of a very concentrated distribution surrounded by a halo distribution appears difficult to understand if all particles had been produced at one ...
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1038/201803a0
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  • 10
    Electronic Resource
    Electronic Resource
    Editorial (1989)
    Springer
    The astronomy and astrophysics review 1 (1989), S. 1-1 
    Details
    ISSN: 1432-0754
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1007/BF00872482
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